The SINS/zC-SINF survey of z~2 galaxy kinematics: Evidence for powerful AGN-driven nuclear outflows in massive star-forming galaxies
We report the detection of ubiquitous powerful nuclear outflows in massive (> 10^11 Msun) z~2 star-forming galaxies (SFGs), which are plausibly driven by an Active Galactic Nucleus (AGN). The sample consists of the eight most massive SFGs from our SINS/zC-SINF survey of galaxy kinematics with the...
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| creator | ster Schreiber, N M Genzel, R Newman, S F Kurk, J D Lutz, D Tacconi, L J Wuyts, S Bandara, K Burkert, A Buschkamp, P Carollo, C M Cresci, G Daddi, E Davies, R Eisenhauer, F Hicks, E K S Lang, P Lilly, S J Mainieri, V Mancini, C Naab, T Peng, Y Renzini, A Rosario, D K Shapiro Griffin Shapley, A E Sternberg, A Tacchella, S Vergani, D Wisnioski, E Wuyts, E Zamorani, G |
| description | We report the detection of ubiquitous powerful nuclear outflows in massive (> 10^11 Msun) z~2 star-forming galaxies (SFGs), which are plausibly driven by an Active Galactic Nucleus (AGN). The sample consists of the eight most massive SFGs from our SINS/zC-SINF survey of galaxy kinematics with the imaging spectrometer SINFONI, six of which have sensitive high-resolution adaptive optics (AO) assisted observations. All of the objects are disks hosting a significant stellar bulge. The spectra in their central regions exhibit a broad component in Halpha and forbidden [NII] and [SII] line emission, with typical velocity FWHM ~ 1500 km/s, [NII]/Halpha ratio ~ 0.6, and intrinsic extent of 2 - 3 kpc. These properties are consistent with warm ionized gas outflows associated with Type 2 AGN, the presence of which is confirmed via independent diagnostics in half the galaxies. The data imply a median ionized gas mass outflow rate of ~ 60 Msun/yr and mass loading of ~ 3. At larger radii, a weaker broad component is detected but with lower FWHM ~ 485 km/s and [NII]/Halpha ~ 0.35, characteristic for star formation-driven outflows as found in the lower-mass SINS/zC-SINF galaxies. The high inferred mass outflow rates and frequent occurrence suggest the nuclear outflows efficiently expel gas out of the centers of the galaxies with high duty cycles, and may thus contribute to the process of star formation quenching in massive galaxies. Larger samples at high masses will be crucial to confirm the importance and energetics of the nuclear outflow phenomenon, and its connection to AGN activity and bulge growth. |
| doi_str_mv | 10.48550/arxiv.1311.2596 |
| format | Article |
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The sample consists of the eight most massive SFGs from our SINS/zC-SINF survey of galaxy kinematics with the imaging spectrometer SINFONI, six of which have sensitive high-resolution adaptive optics (AO) assisted observations. All of the objects are disks hosting a significant stellar bulge. The spectra in their central regions exhibit a broad component in Halpha and forbidden [NII] and [SII] line emission, with typical velocity FWHM ~ 1500 km/s, [NII]/Halpha ratio ~ 0.6, and intrinsic extent of 2 - 3 kpc. These properties are consistent with warm ionized gas outflows associated with Type 2 AGN, the presence of which is confirmed via independent diagnostics in half the galaxies. The data imply a median ionized gas mass outflow rate of ~ 60 Msun/yr and mass loading of ~ 3. At larger radii, a weaker broad component is detected but with lower FWHM ~ 485 km/s and [NII]/Halpha ~ 0.35, characteristic for star formation-driven outflows as found in the lower-mass SINS/zC-SINF galaxies. The high inferred mass outflow rates and frequent occurrence suggest the nuclear outflows efficiently expel gas out of the centers of the galaxies with high duty cycles, and may thus contribute to the process of star formation quenching in massive galaxies. Larger samples at high masses will be crucial to confirm the importance and energetics of the nuclear outflow phenomenon, and its connection to AGN activity and bulge growth.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1311.2596</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Active galactic nuclei ; Adaptive optics ; Galactic evolution ; Galaxies ; Kinematics ; Massive stars ; Object recognition ; Outflow ; Physics - Cosmology and Nongalactic Astrophysics ; Star & galaxy formation ; Star formation ; Stars & galaxies ; Stellar kinematics</subject><ispartof>arXiv.org, 2014-03</ispartof><rights>2014. 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The sample consists of the eight most massive SFGs from our SINS/zC-SINF survey of galaxy kinematics with the imaging spectrometer SINFONI, six of which have sensitive high-resolution adaptive optics (AO) assisted observations. All of the objects are disks hosting a significant stellar bulge. The spectra in their central regions exhibit a broad component in Halpha and forbidden [NII] and [SII] line emission, with typical velocity FWHM ~ 1500 km/s, [NII]/Halpha ratio ~ 0.6, and intrinsic extent of 2 - 3 kpc. These properties are consistent with warm ionized gas outflows associated with Type 2 AGN, the presence of which is confirmed via independent diagnostics in half the galaxies. The data imply a median ionized gas mass outflow rate of ~ 60 Msun/yr and mass loading of ~ 3. At larger radii, a weaker broad component is detected but with lower FWHM ~ 485 km/s and [NII]/Halpha ~ 0.35, characteristic for star formation-driven outflows as found in the lower-mass SINS/zC-SINF galaxies. The high inferred mass outflow rates and frequent occurrence suggest the nuclear outflows efficiently expel gas out of the centers of the galaxies with high duty cycles, and may thus contribute to the process of star formation quenching in massive galaxies. Larger samples at high masses will be crucial to confirm the importance and energetics of the nuclear outflow phenomenon, and its connection to AGN activity and bulge growth.</description><subject>Active galactic nuclei</subject><subject>Adaptive optics</subject><subject>Galactic evolution</subject><subject>Galaxies</subject><subject>Kinematics</subject><subject>Massive stars</subject><subject>Object recognition</subject><subject>Outflow</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Star & galaxy formation</subject><subject>Star formation</subject><subject>Stars & galaxies</subject><subject>Stellar kinematics</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><sourceid>GOX</sourceid><recordid>eNotkDtvwjAUha1KlYooe6fqSp0D9nWcRzeEgCIhOsAemcSmpnlQOwmPoVN_eEPpdIbz0NFHyBOjQz8Sgo6kPZl2yDhjQxRxcEd6yDnzIh_xgQyc21NKMQhRCN4jP5sPBevFaj26TLxOZ-Aa26ozVBou3wg7mcvTGT5NqQpZm9S9wrQ1mSpTBbqycKiOyuomh_F85WXWtKqEsklzJS1UTa3z6ujAlFBI5zoTXC2t1xULU-5u40a5R3KvZe7U4F_7ZDObbiZv3vJ9vpiMl54ULPS0UDLWvuQsDraBQOQaM8lCX2x9wbM4ZVywLI22Og0wkpRqhhj5ImMiyMKQ8j55vs3-EUoO1hTSnpMrqeRKqgu83AIHW301ytXJvmps2V1KkEYYc8FZyH8B6dhr8Q</recordid><startdate>20140327</startdate><enddate>20140327</enddate><creator>ster Schreiber, N M</creator><creator>Genzel, R</creator><creator>Newman, S F</creator><creator>Kurk, J D</creator><creator>Lutz, D</creator><creator>Tacconi, L J</creator><creator>Wuyts, S</creator><creator>Bandara, K</creator><creator>Burkert, A</creator><creator>Buschkamp, P</creator><creator>Carollo, C M</creator><creator>Cresci, G</creator><creator>Daddi, E</creator><creator>Davies, R</creator><creator>Eisenhauer, F</creator><creator>Hicks, E K S</creator><creator>Lang, P</creator><creator>Lilly, S J</creator><creator>Mainieri, V</creator><creator>Mancini, C</creator><creator>Naab, T</creator><creator>Peng, Y</creator><creator>Renzini, A</creator><creator>Rosario, D</creator><creator>K Shapiro Griffin</creator><creator>Shapley, A E</creator><creator>Sternberg, A</creator><creator>Tacchella, S</creator><creator>Vergani, D</creator><creator>Wisnioski, E</creator><creator>Wuyts, E</creator><creator>Zamorani, G</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20140327</creationdate><title>The SINS/zC-SINF survey of z~2 galaxy kinematics: Evidence for powerful AGN-driven nuclear outflows in massive star-forming galaxies</title><author>ster Schreiber, N M ; 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The high inferred mass outflow rates and frequent occurrence suggest the nuclear outflows efficiently expel gas out of the centers of the galaxies with high duty cycles, and may thus contribute to the process of star formation quenching in massive galaxies. Larger samples at high masses will be crucial to confirm the importance and energetics of the nuclear outflow phenomenon, and its connection to AGN activity and bulge growth.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1311.2596</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Active galactic nuclei Adaptive optics Galactic evolution Galaxies Kinematics Massive stars Object recognition Outflow Physics - Cosmology and Nongalactic Astrophysics Star & galaxy formation Star formation Stars & galaxies Stellar kinematics |
| title | The SINS/zC-SINF survey of z~2 galaxy kinematics: Evidence for powerful AGN-driven nuclear outflows in massive star-forming galaxies |
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